
3C 371 - Wikipedia
3C 371 is a BL Lac object [1] [2] located in the constellation Draco. With a redshift of 0.051, [2] this active galaxy is about 730 million light-years away. [3] 3C 371 is a well known object, first …
[2403.18045] Optical variability of the blazar 3C 371: from minute …
2024年3月26日 · The goal of this study is evaluating the optical variability of 3C 371. Taking advantage of the remarkable cadence of \textit{TESS} data, we aim to characterize the intra …
Multi-wavelength picture of the misaligned BL Lac object 3C 371
2024年12月5日 · Abstract: The BL Lac object 3C 371 is one of the targets that are regularly monitored by the Whole Earth Blazar Telescope (WEBT) Collaboration to study blazar …
Variability studies of 3C 371 - NASA Technical Reports Server (NTRS)
The compact extragalactic radio source, 3C 371, was observed with the X-ray detectors of the EXOSAT satellite for 19.5 hours in 2 observing periods separated by 18 days. This resulted in …
[astro-ph/9912521] Space VLBI Observations of 3C371 - arXiv.org
1999年12月27日 · Abstract: We present the first space VLBI observations of 3C~371, carried out at a frequency of 4.8 GHz. The combination of the high resolution provided by the orbiting …
Optical variability of the blazar 3C 371: From minute to year ...
The BL Lac object 3C 371 was observed by the Transiting Exoplanet Survey Satellite (TESS) for approximately a year, between July 2019 and July 2020, with an unmatched two-minute …
The Double-lobed Blazar 3C 371 - ADS - NASA/ADS
High dynamic range VLA imaging reveals, for the first time, that the blazar 3C 371 exhibits very low surface brightness twin radio lobes. These lobes straddle the dominant compact core and …
Optical variability of the blazar 3C 371: From minute to year ...
2024年6月14日 · The goal of this study is to evaluate the optical variability of 3C 371. Taking advantage of the remarkable cadence of TESS data, we aim to characterize the intra-day …
EXOSAT observations of 3C 371 - NTRS - NASA Technical Reports …
The N galaxy/BL Lacertae object 3C 371 was observed by EXOSAT on two occasions separated by 18 days in September 1984. The low-energy and medium-energy X-ray flux has varied on …
The goal of this study is to evaluate the optical variability of 3C 371. Taking advantage of the remarkable cadence of TESS data, we aim to characterize the intra-day variability (IDV) …
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